𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The centre-to-limb variation of the moon's brightness at 2 and 6cm wavelength

✍ Scribed by W. Hirth; M. Butz; L. Velden; E. Fürst


Publisher
Springer Netherlands
Year
1977
Tongue
English
Weight
249 KB
Volume
17
Category
Article
ISSN
1573-0794

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Brightness temperatures of the quiet sun
✍ E. E. Reber 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 613 KB

Absolute brightness temperatures and brightness temperature ratios of a quiet region near the center of the solar disk and the central region of the new moon were measured simultaneously at the 6 mm wavelength. The measured quiet sun/new moon brightness temperature ratios and reported central bright

On the centre-to-limb variation and lati
✍ P. N. Brandt; E. H. Schröter 📂 Article 📅 1982 🏛 Springer 🌐 English ⚖ 899 KB

Low noise photoelectric measurements of the line profile of the g = 0 Fe line 2 5576.097 combined with determinations of the wavelength shift of its centre calibrated by use of an 12 absorption tube are reported. Measurements taken at various limb distances (1.0 < cos ~ < 0.2) and along 4 different

Shapes and centre-to-limb variation of t
✍ R. B. Teplitskaja; N. M. Firstova 📂 Article 📅 1976 🏛 Springer 🌐 English ⚖ 614 KB

The shapes of the Ca ii H and K lines in sunspot umbral spectra vary from single asymmetric peaks near the centre of the disk to almost symmetric double peaks at the limb. In addition, there are other differences in the behaviour of both H and K lines in sunspots compared to the quiet Sun. The whole

Observation of the absolute intensity an
✍ Keizo Nishi 📂 Article 📅 1973 🏛 Springer 🌐 English ⚖ 443 KB

The absolute intensities and the centre-to-limb variations of the Sun at three wavelengths of 1629 ~, 1684/k, and 1739 ~ were measured by a rocket-borne spectrometer flown from the Kagoshirna Space Centre on 1 September 1971. The spectrometer was a double-dispersive trichrometer, whose spectral and